SDO HMI 2011-11-14 00:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.28 | 105.47 | 30.56 | 249.71 | -17.25 | 105.96 | 76.23 | 251.58 | 0.9768 | -26.6 | 51.8 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.98 | 62.11 | 5.51 | 170.83 | -16.81 | 108.11 | 78.38 | 252.32 | 0.9850 | -294.1 | 66.3 | |
| 4.04 | -1.00 | 10.89 | -1.00 | -16.72 | 107.68 | 77.94 | 252.35 | 0.9837 | 326.8 | 999999 | |
| 0.00 | 5.59 | 0.00 | 15.43 | -18.58 | 107.76 | 78.02 | 250.49 | 0.9846 | 235.0 | 185.7 | |
| 1.81 | 4.73 | 4.50 | 11.74 | -18.55 | 106.53 | 76.80 | 250.38 | 0.9808 | 404.4 | 327.6 | |
| 0.00 | 1.89 | 0.00 | 4.07 | -18.76 | 104.61 | 74.87 | 249.92 | 0.9743 | 139.0 | 85.7 | |
| 0.00 | 1.12 | 0.00 | 2.11 | -19.00 | 102.49 | 72.75 | 249.38 | 0.9660 | 254.0 | 302.5 | |
| 0.00 | 2.15 | 0.00 | 3.72 | -18.67 | 101.00 | 71.26 | 249.49 | 0.9592 | -270.0 | -77.6 | |
| 0.00 | 7.66 | 0.00 | 11.84 | -18.24 | 98.91 | 69.18 | 249.58 | 0.9486 | 296.0 | 156.2 | |
| 3.18 | 7.23 | 4.64 | 10.59 | -17.18 | 97.86 | 68.13 | 250.51 | 0.9420 | -491.0 | -165.3 | |
| 2.67 | 6.19 | 4.09 | 9.53 | -18.86 | 98.67 | 68.93 | 248.90 | 0.9479 | -386.8 | -242.5 | |
| 0.00 | 0.95 | 0.00 | 1.51 | -19.50 | 99.25 | 69.52 | 248.34 | 0.9515 | -262.0 | -250.8 | |
| 0.60 | -10.00 | 0.93 | -10.00 | -19.12 | 98.72 | 68.98 | 248.64 | 0.9485 | -351.6 | 999999 | |
| 0.00 | 5.08 | 0.00 | 7.13 | -17.30 | 97.04 | 67.30 | 250.24 | 0.9375 | -763.0 | -540.1 | |
| 0.00 | 0.77 | 0.00 | 1.21 | -19.51 | 98.91 | 69.17 | 248.27 | 0.9498 | -225.0 | -289.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |